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A Proposed Site for Future Exploration in Libya Montes
The Libya Montes are a highland terrain on Mars up-lifted by the giant impact that created the Isidis basin to the north.
NASA/JPL/University of Arizona (273 km above the surface, less than 5 km top to bottom and north is to the right.)
Source: www.uahirise.org/ESP_022970_1835
Mounds West of Schiaparelli Crater – The mounds seem to have a massive core: possible igneous or mud stocks?
NASA/JPL/University of Arizona (265 km above the surface, less than 1 km top to bottom and North is to the right.) www.uahirise.org/ESP_050216_1730
Possible Fan in a Crater on the Northwestern Rim of the Ladon Valles Basin — This fan form and exposures of light-toned deposits on located on the eastern rim of an unnamed crater.
NASA/JPL/University of Arizona (263 km above the surface. Scene is 5 km across.)
An Unusual Sand Sheet in the Southern Mid-Latitudes — Are these ripples in the sand sheet active? These features are usually found further south, so what are they doing here?
(NASA/JPL/University of Arizona. Acquired: Feb 2017, approximately 249 kilometers above the surface. www.uahirise.org/ESP_049514_1125)
Superb Clay Stratigraphy Northwest of Hellas Planitia — There are also excellent exposures of bedrock in this image.
NASA/JPL/University of Arizona (272 km above the surface and north is to the right.)
Ridges in Meridiani Planum —
These ridges are concentric around an impact crater (not visible in this image.)
NASA/JPL/University of Arizona. (Acquired: Feb 2017, approximately 308 kilometers above the surface, less than 1 km top to bottom and North is to the left. www.uahirise.org/ESP_049557_1835)
How Gas Carves Channels –
The ground likely started as polygonal patterned ground, and then escaping gas widened the channels.
NASA/JPL/University of Arizona (less than 1 km across; www.uahirise.org/ESP_046845_0975)
Lava in Athabasca Valles – It’s not recent, of course, but the lava still has left its mark across an expanse of time.
NASA/JPL/University of Arizona (Mar 2017, 276 km above the surface. Scene is 5 km across. www.uahirise.org/ESP_049736_1880)
The Floor of Burroughs Crater
NASA/JPL/University of Arizona (Acquired: Feb 2017, approximately 250 kilometers above the surface. www.uahirise.org/ESP_049395_1075)
Blocky Deposit along Melas Chasma Floor
NASA/JPL/University of Arizona (Feb 2017, 289 km above the surface. Scene is 5 km across. www.uahirise.org/ESP_049652_1680)
Ancient Rivers: Early in Martian history, liquid water energetically carved the surface, forming channel systems that look remarkably similar to river valleys and drainage networks on Earth. (NASA/JPL/University of Arizona)
Sedimentary and Linear Features Near a Crater Wall
NASA/JPL/University of Arizona (Mar 2017, 253 km above the surface. Scene is 5 km across. www.uahirise.org/ESP_049712_1525)
Bedrock Outcrops in Kaiser Crater – The wind has stripped off the overlying soil, and created grooves and scallops in the bedrock.
NASA/JPL/University of Arizona (www.uahirise.org/ESP_012239_1330)
Tripping the Dune Fantastic!
NASA/JPL/University of Arizona (Acquired: Feb 2017, approximately 268 kilometers above the surface. www.uahirise.org/ESP_049362_1295)
The Entrance to Mawrth Vallis – Driving over this terrain will be much more difficult than it was depicted in the novel, "The Martian."
NASA/JPL/University of Arizona (www.uahirise.org/ESP_049017_2060)
Rounded Mounds in Northern Arabia Terra: The resolution of our image will help assess the nature and grain size of the sediment that makes up these mounds.
Image: NASA/JPL/University of Arizona
Fotografías realizadas por Laura León para el proyecto Eurovelo 1. Las imágenes solo podrán ser utilizadas para los fines contratados.
A Small Channel Wriggles Away from a Crater in Phlegra Montes
NASA/JPL/University of Arizona (Mar 2017, 312 km above the surface. Scene is 5 km across. www.uahirise.org/ESP_049709_2185)
Crater Wall Art
NASA/JPL/University of Arizona (Acquired: Nov 2016, 251 km above the surface. Scene is 5 km top to bottom and North is approximately to the right. www.uahirise.org/ESP_048488_1285)
Old Salt: Just what is that "purplish" colored stuff with the polygonal fractures? (www.uahirise.org/ESP_044502_1735)
Small Crater Exposed in Cross-Section by Erosion
Image: NASA/JPL/University of Arizona (Approximately 5 km across. www.uahirise.org/ESP_016699_1715)
Photograph taken at 13:29pm on August 19th 2010 in Friezland Wood, overlooking Fairview Lane at the High Rocks, Tunbridge Wells, Kent, England.
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Model: Janine Curties
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Nikon D700 50mm 1/30s f/5.6 iso200 Handheld. Manual exposure. Af-s single point focus. Matrix metering.
Nikkor 50mm f/1.8D AF. UV filter
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RAW (TIFF) FILE SIZE: 54.00MB
PROCESSED (JPeg) SIZE: 4.69MB
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PROCESSING POWER:
Nikon D700 Firmware versions A 1.10 B 1.10 L 2.009 (Lens distortion control version 2)
HP 110-352na Desktop PC with AMD Quad-Core A6-5200 APU processor. AMD Radeon HD8400 graphics. 8 GB DDR3 Memory with 1TB SATA storage. 64-bit Windows 10. Verbatim USB 2.0 1TB desktop hard drive. WD My Passport Ultra 1tb USB3 Portable hard drive. Nikon ViewNX-1 64bit (Version 1.2.4 24/11/2016). Adobe photoshop Elements 8 Version 8.0 64bit.
Intracrater Buttes — This is an interesting candidate for an ancient landslide lobe, light-toned materials, buttes, buttes with summit pits, retreating scarps…just about everything is here!
NASA/JPL/University of Arizona (259 km above the surface, 5 km across.)
Spiders on Ejecta Blankets – These are not actual spiders, of course, but the term given to the shape of the darker, exposed subsurface material that results from sublimation, when a solid goes directly into a gaseous state.
NASA/JPL/University of Arizona (Acquired: November 2016, approximately 250 kilometers above the surface. Scene is 5 km across. www.uahirise.org/ESP_048451_1010)
Unfilled Circular Depression with Possible Clay Signatures
NASA/JPL/University of Arizona (Acquired: November 2016, approximately 249 kilometers above the surface. Scene is 5 km across; www.uahirise.org/ESP_048137_1510)
Faulted and Stratified Rock in a Crater to the East of Schiaparelli Crater — There are possible incipient landslides off the flank of this crater-hosted mound of stratified rock. It’s also a good opportunity to study landslide structure in stratified rocks.
NASA/JPL/University of Arizona (266 km above the surface, 5 km across.)
A Mass of Viscous Flow Features – Viscous, lobate flow features are commonly found at the bases of slopes in the mid-latitudes of Mars, and are often associated with gullies.
NASA/JPL/University of Arizona (www.uahirise.org/ESP_048913_1330)
Possible Clay Deposits in Libya Montes
NASA/JPL/University of Arizona (267 km above surface and the scene is 5 km across.)
Terrain West of the Clay-Bearing Units of Mawrth Vallis
NASA/JPL/University of Arizona (5 km across, www.uahirise.org/ESP_013849_2030)
Southern Wall of a Canyon-Like Structure
NASA/JPL/University of Arizona (Apr 2011, 255 km above the surface, 5 km across; www.uahirise.org/ESP_022080_1690)
Possible Olivine-Rich Terrain on Etched, Intercrater Plains
NASA/JPL/University of Arizona (Dec 2009, 264 km above the surface, 5 km across; www.uahirise.org/ESP_015969_1775)
LIght-Toned Bedrock along the Floor of Coprates Catena
NASA/JPL/University of Arizona (5 km across; www.uahirise.org/ESP_019903_1645)
Yardangs: Nature’s Weathervanes
Though often beautiful to look at, yardangs are not permanent and will be eroded away by the persistence of the Martian winds.
NASA/JPL/University of Arizona (uahirise.org/ESP_050420_1910)
Terrain between South and Main Craters (Almost sounds like an address.)
NASA/JPL/University of Arizona (Nov 2016, 250 km above the surface, 5 km across; www.uahirise.org/ESP_048172_1025)
Slope Monitoring
NASA/JPL/University of Arizona (Acquired: Nov 2016, 279 km above the surface. Scene is 5 km across. www.uahirise.org/ESP_048490_1695)
Charlis Ortíz en el compromiso que enfrentó a Real Esppor Club y Trujillanos Fútbol Club, en el estadio nacional Brígido Iriarte (Nelson Pulido)
The Plains are Not Plain – This image covers some of the plains south of Capri Chasma in eastern Valles Marineris. (www.uahirise.org/ESP_045300_1630)
Cryptic Terrain – We call it “cryptic” only because of the lack of easily identifiable features.
NASA/JPL/University of Arizona (Nov 2016, 249 km above the surface, 5 km across; www.uahirise.org/ESP_048169_0985)
Southern Intercrater Plains
NASA/JPL/University of Arizona (Nov 2016, 250 km above the surface, 5 km across; www.uahirise.org/ESP_048167_1165)